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researcher

M. Arnaboldi

10 papers hereh-index 176 citations5 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author2
  • middle author7

Across the 10 of 10 papers where every author was matched, so the position is known.

fields
  • astro-ph6
  • astro-ph.GA3
  • astro-ph.CO1
same name
  • M. Arnaboldi — 127 papers, h 41
  • M. Arnaboldi — 56 papers, h 25
  • M. Arnaboldi — 17 papers, h 4
  • M. Arnaboldi — 1 paper
  • M. Arnaboldi — 1 paper, h 14
  • M. Arnaboldi — 1 paper, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19972026
most citedThe Planetary Nebulae Spectrograph: the green light for Galaxy Kinematics

101 citations · 336 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2026

Kinematically cold and warm planetary nebulae samples, HII regions and supernovae remnants in the disc of the face-on spiral galaxy NGC 628 (M74) -- The Planetary Nebulae Spectrograph with the Hα arm

Magda Arnaboldi, Ortwin Gerhard, Surya Aniyan +14

We present the results for the galaxy NGC 628 observed with the Planetary Nebulae Spectrograph (PN.S) equipped with the Hα arm. With the third PN.S arm, the Hα arm, we measure…

astro-ph.GA2023★ 7 cited

The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs

C. Pulsoni, O. Gerhard, S. M. Fall +5

Mass and angular momentum are key parameters of galaxies. Their co-evolution establishes an empirical relation between the specific stellar angular momentum j* and the stellar mass…

astro-ph.GA2011★ 43 cited

Unravelling the origins of S0 galaxies using maximum likelihood analysis of planetary nebulae kinematics

A. Cortesi, M. R. Merrifield, M. Arnaboldi +12

To investigate the origins of S0 galaxies, we present a new method of analyzing their stellar kinematics from discrete tracers such as planetary nebulae. This method involves binni…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.